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http://hub.abes.fr/edp/periodical/aa/2016/volume_590/issue_2016/aa27718-15/authorship/3
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Mass loss from inhomogeneous hot star winds
Atmospheric NLTE models for the spectroscopic analysis of blue stars with winds
Determining the effects of clumping and porosity on the chemistry in a non-uniform AGB outflow (Corrigendum)
Atmospheric NLTE models for the spectroscopic analysis of blue stars with winds
Radiography in high mass X-ray binaries
Analytic, dust-independent mass-loss rates for red supergiant winds initiated by turbulent pressure
Shock-heated radiation-driven outflows as a solution to the weak-wind problem of late O-type stars
Constraining the overcontact phase in massive binary evolution
Empirical mass-loss rates and clumping properties of Galactic early-type O supergiants
Simulations of the line-driven instability in magnetic hot star winds
Upper mass-loss limits and clumping in the intermediate and outer wind regions of OB stars
Binary-object spectral-synthesis in 3D (BOSS-3D)
The R136 star cluster dissected with Hubble Space Telescope/STIS
Theoretical wind clumping predictions from 2D LDI models of O-star winds at different metallicities
The dusty circumstellar environment of Betelgeuse during the Great Dimming as seen by VLTI/MATISSE
New predictions for radiation-driven, steady-state mass-loss and wind-momentum from hot, massive stars
Mass loss from inhomogeneous hot star winds
The rotation rates of massive stars
Mass loss from inhomogeneous hot star winds
Long term variability of Cygnus X-1
2D wind clumping in hot, massive stars from hydrodynamical line-driven instability simulations using a pseudo-planar approach
3D radiative transfer: Continuum and line scattering in non-spherical winds from OB stars
Determining the effects of clumping and porosity on the chemistry in a non-uniform AGB outflow
Atmospheric NLTE models for the spectroscopic analysis of blue stars with winds
Formation of wind-captured disks in supergiant X-ray binaries
Wind Roche lobe overflow in high-mass X-ray binaries
Theoretical wind clumping predictions of OB supergiants from line-driven instability simulations across the bi-stability jump
New predictions for radiation-driven, steady-state mass-loss and wind-momentum from hot, massive stars
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